activity
20132026
most citedA kilonova as the electromagnetic counterpart to a gravitational-wave source

888 citations · 3k across the 88 of their papers we have counts for

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Showing 2019Show all

8 papers · 1 filter

astro-ph.HE2019

Calibrating the power of relativistic jets

L. Foschini, M. L. Lister, T. Hovatta +12

There are several methods to calculate the radiative and kinetic power of relativistic jets, but their results can differ by one or two orders of magnitude. Therefore, it is necess…

astro-ph.GA2019★ 13 cited

Broadband X-ray observations of four gamma-ray narrow-line Seyfert 1 galaxies

M. Berton, V. Braito, S. Mathur +4

Narrow-line Seyfert 1 galaxies (NLS1s) is one of the few classes of active galactic nuclei (AGN) harboring powerful relativistic jets and detected in rays. NLS1s are well-known…

astro-ph.GA2019

A correlation between [O III] line property and X-ray spectral complexity in narrow-line Seyfert 1 galaxies?

S. Chen, G. La Mura, M. Berton +7

We present a detailed study of 11 narrow-line Seyfert 1 galaxies (NLS1s) from the Six-degree Field Galaxy Survey (6dFGS) that both have optical and X-ray spectroscopic observations…

astro-ph.GA2019★ 12 cited

Line shapes in narrow-line Seyfert 1 galaxies: a tracer of physical properties?

M. Berton, I. Björklund, A. Lähteenmäki +4

Line profiles can provide fundamental information on the physics of active galactic nuclei (AGN). In the case of narrow-line Seyfert 1 galaxies (NLS1s) this is of particular import…

astro-ph.GA2019

Mapping the narrow-line Seyfert 1 galaxy 1H 0323+342

Luigi Foschini, Stefano Ciroi, Marco Berton +3

Taking advantage of the most recent measurements by means of high-resolution radio observations and other multiwavelength campaigns, it is possible to elaborate a detailed map of t…

astro-ph.HE2019★ 53 cited

SN 2017gmr: An energetic Type II-P supernova with asymmetries

Jennifer E. Andrews, D. J. Sand, S. Valenti +77

We present high-cadence ultraviolet (UV), optical, and near-infrared (NIR) data on the luminous Type II-P supernova SN 2017gmr from hours after discovery through the first 180 days…